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Structure of Galaxies Embedded in Clouds of Dark Matter

Published online by Cambridge University Press:  03 August 2017

R. Cowsik
R. Cowsik*
Affiliation:
Tata Institute of Fundamental Research, Bombay 400 005

Abstract

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The purpose of this poster is to draw attention to the recent papers of Cowsik and Ghosh (J.A.A. 7, 7, 1986 et seq. and Ap.J., 317, 26, 1987) where particles of dark matter, stars and galaxies are treated as collissionless gasses. The encounterless Boltzmann equations become coupled through the common gravitational potential in which they move. Assuming that the distributions have the Maxwellian or generalised Schwarzschild form, the potentials ϕg, ϕv due to the baryonic and dark matter are shown to satisfy the coupled equations:

Type
Appendix 1: Poster Papers
Information
Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 589
Copyright
Copyright © Reidel 1988